Magnetic Properties and Paleomagnetism of Zebra Rock, Western Australia: Chemical Remanence Acquisition in Hematite Pigment and Ediacaran Geomagnetic Field Behavior
dc.contributor.author | Abrajevitch, Alexandra | |
dc.contributor.author | Pillans, Bradley | |
dc.contributor.author | Roberts, Andrew P. | |
dc.contributor.author | Kodama, Kazuto | |
dc.date.accessioned | 2021-11-15T23:01:24Z | |
dc.date.available | 2021-11-15T23:01:24Z | |
dc.date.issued | 2018 | |
dc.date.updated | 2020-11-23T11:47:18Z | |
dc.description.abstract | Zebra Rock, a decorative stone remarkable for its unusual pattern of regularly spaced reddish bands and rods with white background, is found within the Neoproterozoic succession in East Kimberley, Western Australia. The unusual pigment distribution suggests that precipitation of hematite, or its precursor phase, occurred in a single episode. Magnetic properties of hematite pigment in Zebra Rock are distinctly different from those of the host shale, with a smaller median particle size and higher degree of structural perfection. The low thermal stability of the Zebra Rock pigment, with onset of thermal alteration at 300°C, suggests that the rocks have not undergone significant metamorphic heating. Stepwise thermal demagnetization reveals multiple magnetization components. Short-range variability in the relative contributions of the components to the total remanence is indicative of the stochastic nature of the hematite pigment growth process. In addition to seven magnetization components with shallow to intermediate inclinations that can be matched to the Paleozoic Australian apparent polar wander path, Zebra Rock samples contain a distinct steeply dipping magnetization that is not observed in the host shales. The steep magnetization appears to be primary, based on its unique association with the Zebra pattern, dissimilarity with younger directions, and evidence for low degree of thermal alteration of the rocks. The steep characteristic remanence contrasts with previous paleomagnetic indications of low Australian Neoproterozoic paleolatitudes. The characteristic Zebra Rock magnetization is the first Australian example of incompatible magnetization directions that have been reported previously from Ediacaran rocks in Laurentia, Baltica, and Africa. | en_AU |
dc.description.sponsorship | We acknowledge the Australian Research Council (ARC) through grant FS100100076 to APR and colleagues that provided a Super Science Fellowship to AA. | en_AU |
dc.format.mimetype | application/pdf | en_AU |
dc.identifier.issn | 1525-2027 | en_AU |
dc.identifier.uri | http://hdl.handle.net/1885/251827 | |
dc.language.iso | en_AU | en_AU |
dc.provenance | https://v2.sherpa.ac.uk/id/publication/11055..."The Published Version can be archived in Institutional Repository. 6 months embargo" from SHERPA/RoMEO site (as at 16/11/2021). An edited version of this paper was published by AGU. Copyright (2018) American Geophysical Union | en_AU |
dc.publisher | American Geophysical Union | en_AU |
dc.relation | http://purl.org/au-research/grants/arc/FS100100076 | en_AU |
dc.rights | © 2018. American Geophysical Union. | en_AU |
dc.source | Geochemistry, Geophysics, Geosystems | en_AU |
dc.title | Magnetic Properties and Paleomagnetism of Zebra Rock, Western Australia: Chemical Remanence Acquisition in Hematite Pigment and Ediacaran Geomagnetic Field Behavior | en_AU |
dc.type | Journal article | en_AU |
dcterms.accessRights | Open Access | en_AU |
local.bibliographicCitation.issue | 3 | en_AU |
local.bibliographicCitation.lastpage | 748 | en_AU |
local.bibliographicCitation.startpage | 732 | en_AU |
local.contributor.affiliation | Abrajevitch, Alexandra, College of Science, ANU | en_AU |
local.contributor.affiliation | Pillans, Bradley, College of Science, ANU | en_AU |
local.contributor.affiliation | Roberts, Andrew, College of Science, ANU | en_AU |
local.contributor.affiliation | Kodama, Kazuto, Kochi University | en_AU |
local.contributor.authoremail | u4817957@anu.edu.au | en_AU |
local.contributor.authoruid | Abrajevitch, Alexandra, t1384 | en_AU |
local.contributor.authoruid | Pillans, Bradley, u9400437 | en_AU |
local.contributor.authoruid | Roberts, Andrew, u4817957 | en_AU |
local.description.notes | Imported from ARIES | en_AU |
local.identifier.absfor | 040299 - Geochemistry not elsewhere classified | en_AU |
local.identifier.absfor | 040499 - Geophysics not elsewhere classified | en_AU |
local.identifier.ariespublication | a383154xPUB9551 | en_AU |
local.identifier.citationvolume | 19 | en_AU |
local.identifier.doi | 10.1002/2017GC007091 | en_AU |
local.identifier.scopusID | 2-s2.0-85043515094 | |
local.identifier.uidSubmittedBy | a383154 | en_AU |
local.publisher.url | http://sites.agu.org/ | en_AU |
local.type.status | Published Version | en_AU |
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